X. T. Huang
Shandong University
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Featured researches published by X. T. Huang.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999
P. Cennini; J.-P. Revol; C. Rubbia; F. Sergiampietri; A. Bueno; M. Campanelli; P Goudsmit; A. Rubbia; L. Periale; S. Suzuki; C. Chen; Y. X. Chen; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Xu; Z. Xu; C. C. Zhang; Qingmin Zhang; S.C. Zheng; F. Cavanna; D. Mazza; G. Piano Mortari; S. Petrera; C. Rossi; G. Mannocchi; P. Picchi; F. Arneodo
A system to detect light from liquid argon scintillation has been implemented in a small, ICARUS-like, liquid argon time projection chamber. The system, which uses a VUV-sensitive photomultiplier to collect the light, has recorded many ionizing tracks from cosmic-rays in coincidence with scintillation signals. Our measurements demonstrate that scintillation light detection can provide an effective method for absolute time measurement of events and eventually a useful trigger signal
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2000
F. Arneodo; A. Badertscher; S Baibussinov; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; D. Cline; I. De Mitri; R. Dolfini; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Mannocchi; M Maris
Abstract The ICARUS time projection chamber can yield sound information on 8 B solar neutrinos. Owing to the high-energy resolution and the good capability of event reconstruction it can make a contribution to our understanding of neutrino intensities and their energy spectrum. Moreover, the MSW oscillation probability for sterile and active neutrinos can be well studied because both elastic scattering by electrons and absorption reaction on argon nuclei can be measured independently. The main problem in detecting the low-energy neutrino interactions arises from the environmental radioactivity. In the present work we study by Monte Carlo simulation the topology and the rates of the events, induced by neutrinos and background neutrons, in a 470 t (fiducial mass) liquid-argon TPC detector. For neutrino interactions we use the standard solar model BP98 and the recent experimental confirmation of the shell model computation of absorption cross section. The noise is estimated from new data on natural neutron background, collected in the hall C of the Gran Sasso laboratory. It is confirmed that, with a relatively modest neutron shielding and particular off-line event triggers, the weight of spurious events can be made to have little influence on the ICARUS solar neutrino measurement. Indeed, we expect 6 (26) background events per year in the 212 (759) elastic scattering (absorption reaction) sample.
Physical Review D | 2013
M. Ablikim; M. N. Achasov; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. Becker; J. V. Bennett; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; R. A. Briere; V. Bytev; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen; M. L. Chen
The decay
Nuclear Physics B - Proceedings Supplements | 2000
C. Vignoli; F. Arneodo; A. Badertscher; E. Barbieri; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; F. Carli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; C. Cinquini; D. Cline; I. De Mitri; R. Dolfini; D. Favaretto; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li
J/\psi \rightarrow \omega p \bar{p}
Physical Review D | 2013
M. Ablikim; M. N. Achasov; X. C. Ai; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. V. Bennett; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; S. Braun; R. A. Briere; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen; M. L. Chen
has been studied, using
Physical Review D | 2013
M. Ablikim; M. N. Achasov; O. Albayrak; D. J. Ambrose; F. F. An; Q. An; J. Z. Bai; R. Baldini Ferroli; Y. Ban; J. Becker; J. V. Bennett; N. Berger; M. Bertani; J. M. Bian; E. Boger; O. Bondarenko; I. Boyko; R. A. Briere; V. Bytev; H. Cai; X. Cai; O. Cakir; A. Calcaterra; G. F. Cao; S. A. Cetin; J. F. Chang; G. A. Chelkov; G. Chen; H. S. Chen; J. C. Chen
225.3\times 10^{6}
Physical Review Letters | 2012
O. Bondarenko; J. C. Chen; Min Chen; J. P. Dai; Y. Gao; J. S. Huang; X. T. Huang; L. K. Jia; S. L. Jin; N. Kalantar-Nayestanaki; M. Kavatsyuk; J. S. Lange; F. Y. Li; Guihua Li; Haibo B. Li; N. B. Li; S. L. Li; Hao Liang; Y. T. Liang; G. R. Liao; C. L. Liu; C. X. Liu; C. Y. Liu; K. Liu; K. Y. Liu; H. Loehner; J. G. Lu; X. L. Luo; C. L. Ma; J. G. Messchendorp
Physical Review D | 2011
M. Ablikim; M. N. Achasov; O. Bondarenko; J. C. Chen; M. L. Chen; J. P. Dai; Y. Gao; J. S. Huang; X. T. Huang; L. K. Jia; S. Jin; M. Kavatsyuk; J. S. Lange; F. Y. Li; G. Li; H. B. Li; N. B. Li; Hao Liang; Y. T. Liang; G. R. Liao; C. L. Liu; C. X. Liu; C. Y. Liu; G. C. Liu; K. Liu; K. Y. Liu; Z. Q. Liu; H. Loehner; J. G. Lu; X. L. Luo
J/\psi
Physical Review Letters | 2005
M. Ablikim; J. Z. Bai; Y. Ban; J.G. Bian; X. Cai; H.F. Chen; H. S. Chen; H.X. Chen; J. C. Chen; Jin Chen; Y. B. Chen; S.P. Chi; Y. P. Chu; X.Z. Cui; Y.S. Dai; Z. Y. Deng; L. Y. Dong; Q.F. Dong; S. X. Du; Z.Z. Du; J. Fang; S. S. Fang; C. D. Fu; C.S. Gao; Y. Gao; S.D. Gu; Y. T. Gu; Y. Guo; Y. Q. Guo; Z. J. Guo
events accumulated at BESIII. No significant enhancement near the
Physical Review Letters | 2008
M. Ablikim; J. Z. Bai; Y. Bai; Y. Ban; X. Cai; H.F. Chen; H. S. Chen; H.X. Chen; J. C. Chen; Jin Chen; X. Chen; Y. B. Chen; Y. P. Chu; Y.S. Dai; Z. Y. Deng; S. X. Du; J. Fang; C. D. Fu; C.S. Gao; Y. Gao; S.D. Gu; Y. T. Gu; Y. Guo; Z. J. Guo; F. A. Harris; K. L. He; M. He; Y. K. Heng; J. Hou; H. M. Hu
p\bar{p}